Penumbral lunar eclipse of 2020, January 10 The beginning of the eclipse is visible from Eurasia, Alaska, Australia, northeast part of Africa, Madagascar, Arctic, west of Pacific, and Indian oce- ans. The end of the eclipse is visible from Eurasia, Africa, Madagascar, north of North America, Greenland, Arctic, Indian, and Atlantic oceans. Universal time of geocentric opposition h m s in right ascension 2020, January 10, 19 04 13.6 Sun Moon h m s h m s Right ascension . . . . . . . . . . . . . 19 26 30.986 7 26 30.985 s s Hourly motion . . . . . . . . . . . . . +10.865 +153.374 o ' " o ' " Declination. . . . . . . . . . . . . . . . -21 56 51.81 +23 00 14.53 " " Hourly motion . . . . . . . . . . . . . +22.41 -120.75 " ' " Equatorial horizontal parallax . . . . . . 8.94 59 00.63 ' " ' " Apparent semidiameter . . . . . . . . . . 16 15.89 16 04.80 Circumstances of the Eclipse Position Angles of the Moon's axis h m o Moon enters penumbra . . . . . . . January 10, 17 05.7 9.46 Greatest eclipse . . . . . . . . . 19 10.1 9.95 Moon leaves penumbra . . . . . . . 21 14.5 10.44 ----------------------------------------------- Contacts | Position |The Moon being in the Zenith in of penumbra| Angles |------------------------ with Limb | from the | | of Moon |North Point| Latitude | Longitude ----------|-----------|----------|------------- | o ' | o ' | o ' First | 135 20.6 ¦ +23 12.3 ¦ 104 15.5 E Last | 230 30.9 ¦ +23 03.8 ¦ 44 32.0 E Magnitude of the eclipse 0.919 " Angular radius of the penumbra 4615.85 " Angular radius of the umbra 2625.34 ------------------------------------------------------------------------------ T | s | d | P |Magnitudes ofI T | s | d | P |Magnitudes of | | | | penumbral I | | | | penumbral -----|-----|------|------|-------------I-----|-----|------|------|------------ h m¦ "¦ ¦ o ¦ I h m¦ "¦ ¦ o ¦ 17 00¦ 5709¦ 2.177¦ 134.1¦ Д I19 20¦ 3812¦ 1.452¦ 187.9¦ 0.911 10¦ 5468¦ 2.085¦ 136.4¦ 0.054 I 30¦ 3854¦ 1.468¦ 192.8¦ 0.890 20¦ 5238¦ 1.997¦ 138.9¦ 0.173 I 40¦ 3924¦ 1.494¦ 197.6¦ 0.854 30¦ 5018¦ 1.913¦ 141.7¦ 0.287 I 50¦ 4019¦ 1.530¦ 202.1¦ 0.805 40¦ 4810¦ 1.834¦ 144.7¦ 0.395 I ¦ ¦ ¦ ¦ 50¦ 4616¦ 1.760¦ 147.9¦ 0.495 I20 00¦ 4138¦ 1.575¦ 206.5¦ 0.744 ¦ ¦ ¦ ¦ I 10¦ 4279¦ 1.629¦ 210.6¦ 0.672 18 00¦ 4438¦ 1.692¦ 151.4¦ 0.587 I 20¦ 4439¦ 1.690¦ 214.4¦ 0.589 10¦ 4278¦ 1.630¦ 155.2¦ 0.670 I 30¦ 4618¦ 1.758¦ 217.9¦ 0.497 20¦ 4137¦ 1.576¦ 159.3¦ 0.743 I 40¦ 4813¦ 1.832¦ 221.2¦ 0.396 30¦ 4018¦ 1.531¦ 163.7¦ 0.804 I 50¦ 5021¦ 1.911¦ 224.2¦ 0.289 40¦ 3923¦ 1.495¦ 168.2¦ 0.853 I ¦ ¦ ¦ ¦ 50¦ 3854¦ 1.468¦ 173.0¦ 0.889 I21 00¦ 5242¦ 1.995¦ 226.9¦ 0.175 ¦ ¦ ¦ ¦ I 10¦ 5474¦ 2.083¦ 229.4¦ 0.055 19 00¦ 3812¦ 1.452¦ 177.9¦ 0.911 I 20¦ 5715¦ 2.174¦ 231.8¦ Д 10¦ 3798¦ 1.447¦ 182.9¦ 0.919 I ¦ ¦ ¦ ¦ T - universal time ( TDT - UT1 = 70.0s); s - the angular distance between the centers of the Moon and the shadow; d - the linear distance between the Moon's center and that of the shadow in terms of the shadow's radius; P - the position angle of the Moon's disk semi-diameter directed towards the shadow's center.